... Unbiased surveies of star-forming regions; evolutionary processes in star formation; IMF; determination of evolutionary tracers . ... Light elements; mixing in stars . ... Spectroscopy of low-mass stars in SFRs/associations: cluster formation, triggered SF, SFHs, accretion properties . ... Influence of cooling e and magnetic field on the formation of primordial stars . ... This email address is being protected from spambots. You need JavaScript enabled to view it. ... 39 0552752 251 . ...

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• INAF - Arcetri Astrophysical Observatory
• A homogeneous chemical analysis of the inner Galactic disk from the first data
• Dust evolution across the CO snowline in a protoplanetary disk

... Science . ... Science Users Information > Science Activities > Science in Garching . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Understanding the diversity and consequences of star and planet formation is a key area of research for ESO. ... Read more and see who is involved in this research area.. Stellar structure and evolution includes the internal structureof stars, the structure and dynamics of stellar atmospheres,as well as stellar winds and mass-loss. ... ESO . ...

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• ESO - Research Area: STELLAR POPULATIONS
• ESO - Research Area: STELLAR STRUCTURE AND EVOLUTION
• ESO - Research Area: COSMOLOGY AND THE EARLY UNIVERSE

STScI . Research . ... The 8.4m ground-based Large Synoptic Survey Telescope will survey the entire visible sky deeply in multiple colors every week probing dark matter and dark energy, searching for supernovae, near-Earth asteroids and Kuiper-belt Objects. ... GRAPES is an ACS grism spectroscopic survey of the Hubble Ultra Deep Field. ... The Hubble Deep Field is a Director's Discretionary program on HST to image a typical field at high galactic latitude in four wavelengths as deeply as possible. ...

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• GOODS: The Great Observatories Origins Deep Survey
• HST this week: 141
• IAU Symposium 267: Evolution of Galaxies and Central Black Holes

... Australia Telescope Steering Committee . ... Parkes radio telescope . ... Late Stages of Stellar Evolution . Welcome to the home page of the Late Stages of Stellar Evolution" We are a research group which operates within the Astrophysics Group of the Australia Telescope National Facility. ... To investigate the late stages of stellar evolution and in particular the role of stellar mass-loss in the evolution of asymptotic giant branch stars, proto-planetary nebulae and extremely massive stars. ...

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• Local HI: Constraints on the evolution of the HI content of the Universe
• Star formation and gas distribution in the Magellanic Spiral NGC 4214
• Studying Galaxy Evolution: A Galaxy Zoo Conference

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

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• Astrophysical Research Consortium - Apache Point Observatory

... Research interests of Observatory staff currently focus on (i) Stellar and Galactic Astrophysics (including star formation, astrophysical jets, cool stars , hot stars , helium stars , star-spots, stellar flares, circumstellar dust), (ii) the Sun (the dynamic solar atmosphere, chromosphere and corona), (iii) Solar ... A subset of the Armagh Observatory's research activity, namely the list of 34 refereed journal publications during 2003, is given in Appendix C . ... Solar System Astronomy ....

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• Solar System Research
• M.D. Smith, Research Astronomer
• Armagh Observatory

BSc thesis "Metallicity Gradients of Elliptical Galaxies", 1997, Univ. of Tokyo . MSc thesis "Low-Metallicity Inhibition of Type Ia Supernovae and Galactic and Cosmic Chemical Evolution", 1999, Univ. of Tokyo . PhD thesis "Formation and Chemodynamical Evolution of Galaxies", 2002, Univ. of Tokyo . ... Cosmic SFRs, chemical evolution, mass-dependent galactic winds, and the mass-metallicity relation of galaxies are reproduced (Kobayashi, Springel, White 06). ... What are dwarf galaxies? ...

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• RSAA website - Intranet - ANU
• COALA - Computational Astrophysics Laboratory
• Philip Lah's Research

... The observed isotropy on the sky and non-uniform spatial distribution of gamma-ray bursts   (GRB) revealed by the BATSE   device onboard the Compton Gamma-Ray Observatory (e.g. Meegan et al. , 1992)[ 138 ] lend support to the idea of a cosmological origin of GRB (Prilutski and Usov, 1975;[ 165 ] Usov and Chibisov, 1975)[ 199 ] for which the best candidates could be merging binary NS+NS   or NS+BH   at high redshifts (z 1 -2), (Blinnikov et al. ... Calculation of Binary Neutron Star Coalescence Rates...

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• Evolution of the double neutron star merging rate and the cosmological origin
• Effect of sources evolution on
• Introduction

... More recently, I have been concerned with observing masers located in the circumstellar shells generated by red giant stars in their mass-loss phase, and in what we can therefore learn about the late stages of stellar evolution. 100 mJy are now undetectable after ~12 years, aka the DEATH of an OH/IR star or its cyclical evolution back to a Mira variable. ... I find that this momentum flux is sufficient to support the largest observed rates of AGB mass-loss. last updated: 14 January 2015 . ...

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• The Evolution of Galaxies through the Neutral Hydrogen Window The Evolution of
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution
• National Astronomy and Ionosphere Center (Arecibo Observatory)

... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . Dept. for Space Plasma Physics . ... Dept. for Solar Physics . ... 2016,MNRAS, 2016MNRAS.tmp.. ... 2016,MNRAS, Vol.455 ,is.1,p.357-369. ... 2016,MNRAS, Vol.456 ,is.1,p.181-191. ... WASP- 22, WASP-41, WASP- 42 and WASP- 55. ... Mancini L., Ciceri S., Elyiv A.A.,Physical properties of the planetary systems WASP- 45 and WASP- 46 from simultaneous multiband photometry. 2016,MNRAS, Vol.456 ,Is.1,p.990-1002. ...

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• Achievements - Page 4
• Yaroslav S. Yatskiv
• Summer School ?Atmosphere researches. Challenge for Ukraine?

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

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• Group for study of galaxies and cosmology, history
• Astronomical Schools
• Radio galaxies

BNO is in Baksan Gorge at the Northern Caucasus . ... The Baksan Underground Scintillation Telescope (BUST) of volume 3000 cubic centimeters at a depth of more 300 m. The mountainous plant ANDYRCHI to register wide air showers located over BUST on the area 5*10 4 square metres. The complex of surface plants KOVER including a large muon detector, a scintillation telescope and a neutrino monitor meant for studying the hard component of cosmic rays and wide air showers. ...

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• SAO RAS home page
• About SAO RAS
• topic_en

... Laboratory "Structure" was created in 1992 from the temporary scientific group formed in 1988 in SAO RAS. In December 2003 it was transformed into group of Physics and Evolution of Galaxies , which enters into new Laboratory of Extragalactic ASTROPHYSICS and COSMOLOGY. ... Kniazev A.Y. senior researcher, associated foreign member . Kniazeva T.F. junior researcher, associated foreign member . ... Lipovetsky Valentin A. (1945-1996) former leader of the Laboratory . ...

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• Old "Structure" publications
• "Structure" publications in 1996 year
• Russian-Finnish Symposium, Program

... Astrophysics Group . ... Galaxy Formation and Evolution . ... Gas heating and outflows driven by accreting supermassive black holes (quasar phase) may affect the evolution of star formation in their host galaxy. ... The starburst galaxy M82, which expels dust and metal enriched gas out of its disk . ... The interstellar medium (ISM) plays a central role in galaxy evolution, providing the fuel for star formation and also hosting the ?fossil record? of the galaxy formation history. ...

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• Astrophysics Group Research old
• Astrophysics Group Available research projects/areas
• Astrophysics Group Research

Общая Астрономическая Конференция . ... Правила форума . ... Сообщения за день . ... Добро пожаловать на Общая Астрономическая Конференция. ... Форумы общей направленности . Любые вопросы от новичков (просматривают: 17) . ... Общий форум любителей астрономии (просматривают: 7) . ... Новости магазина Starshop.ru . ... Менее астрономические товары (просматривают: 1) . ... Форум исключительно для сообщений об испытаниях астрономической техники. ... Общая Астрономическая Конференция статистика . ...

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... The obtained results lead to the following conclusions: a) the heavy element enrichment had taken place in the Galaxy in a few bursts of its activity rether than in a continuons manner; b) these bursts occured during the callapse of the early Galaxy; c) the star formation had been inhibited in the time of the bursts; d) the metal enrichment did not proceed in the periods of star formation, between these bursts of activity. ...

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• Vladimir Marsakov Publication List
• Zabotin Nikolay
• Space Research Department of Physics Research Institute

E. V. Miletsky, V. G. Ivanov, Y. A. Nagovitsyn, Some properties of latitude-time evolution of local and background solar magnetic fields // Advances in Space Research, 2015, vol. 55, Issue 3, pp. ... PDF] . E. V.Miletsky, V. G.Ivanov, Amplitude-Time Relations at Different Latitudes in the 11-Year Cycle of Solar Activity // Geomagnetism and Aeronomy, 2015, vol. ... V. G. Ivanov, E. V. Miletsky, Width of Sunspot Generating Zone and Reconstruction of Butterfly Diagram // Solar Physics, 2011. vol. ...

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• Pulkovo Observatory
• General description of the database
• Pulkovo Observatory, Laboratory of Radioastrometry and Geodynamics

... SEARCH ASP SITE: Match ALL words Match ANY word . ... Graduate Student Researcher, Lick Observatory, UC Santa Cruz . Randi writes: "When I was in third grade, I didn't know what I wanted to be. ... I decided to become an astronomer because that way I could use electronic instruments and computers to study the natural world." ... Vy writes: "I wanted to be a veternarian as a kid. ... Only later, in high school, did I start thinking that I wanted to be an astronomer." ... search . ...

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• ASP: Responsible Exploration
• ASP: Good Astronomy Activities on the WWW
• ASP: Cosmology: The Origin, Evolution & Ultimate Fate of the Universe

Laboratory of Stellar Physics . ... A study of close binaries with black holes, neutron stars and white dwarfs. ... A study of SS433 - the massive close binary with a black hole in the regime of supercritical accretion . ... A search for intermediate-mass black holes (IMBH). The black holes which are not supermassive black holes observed in quasars, and which were formed not in massive stars. ... A search for new magnetic stars, new CP stars, measurements of magnetic fields in stars . ...

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• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -
• GRB follow-up team

Dr. Randall Smith . ... Research . ... X-ray Astronomy Schools . ... As this expertise applied generally тАУ to research in abundances and turbulence in galaxy clusters, the chemical composition ofthe Galaxy, and the plasmas found in supernova remnants amongst others тАУ it has led to collaborations working in nearly all areas of X-ray astronomy. ... X-ray Spectra : collisional plasma processes, diffuse emission, supernova remnants, X-ray scattering in dust grains . ... Dept. of Astronomy | ...

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• The Chandra Multiwavelength Project (ChaMP)
• Rotation Periods of PMS Stars
• Spectral Energy Distribution: Microquasar LS 5039